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Simulations of antenna response for the Radio Detector of the Pierre Auger Observatory

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    0580162 - FZÚ 2024 RIV IT eng C - Conference Paper (international conference)
    Abreu, A. - Aglietta, M. - Allekotte, I. - Giaccari, U. - Bakalová, Alena - Blažek, Jiří - Boháčová, Martina - Chudoba, Jiří - Ebr, Jan - Hamal, Petr - Janeček, Petr - Juryšek, Jakub - Mandát, Dušan - Müller, Ana Laura - Palatka, Miroslav - Pech, Miroslav - Prouza, Michael - Řídký, Jan - dos Santos, Eva M. Martins - Schovánek, Petr - Stadelmaier, Maximilian Klaus - Tobiška, Petr - Trávníček, Petr - Vícha, Jakub - Yushkov, Alexey … Total 374 authors
    Simulations of antenna response for the Radio Detector of the Pierre Auger Observatory.
    Proceedings of Science. Vol. 424. Trieste: Sissa Medilab srl, 2023, č. článku 042. ISSN 1824-8039.
    [9th International Workshop on Acoustic and Radio EeV Neutrino Detection Activities (ARENA2022). Santiago de Compostela (ES), 07.06.2022-10.06.2022]
    R&D Projects: GA MŠMT LTT18004; GA MŠMT(CZ) EF18_046/0016010; GA MŠMT EF16_013/0001402
    Research Infrastructure: AUGER-CZ II - 90102
    Institutional support: RVO:68378271
    Keywords : ultra-high-energy cosmic rays * AugerPrime
    OECD category: Particles and field physics
    https://pos.sissa.it/424/042/pdf

    After more than 15 years of successful operation, the Pierre Auger Observatory is currently undergoing a major upgrade called AugerPrime. The aim is to study the mass composition of ultra-high-energy cosmic rays. Part of the upgrade program consists in installing a Short Aperiodic Loaded Loop Antenna (SALLA) atop each of the 1660 water-Cherenkov detectors. To obtain an absolute calibration for the SALLA, the frequency and directionally dependent antenna response (or vector effective length) must be known. The characteristics of the SALLA depend on various parameters, most prominent is the considered frequency of reception and the antenna geometry. Moreover, the interaction with the structure elements and the presence of the ground has an impact.
    Permanent Link: https://hdl.handle.net/11104/0348924

     
     
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